SDO HMI 2014-11-20 18:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.53 | 613.94 | 125.13 | 1018.67 | -13.47 | 164.43 | -71.01 | 104.93 | 0.9519 | 232.1 | -184.0 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.26 | 0.00 | 0.34 | -10.40 | 168.57 | -66.87 | 102.18 | 0.9270 | 335.0 | 272.0 | |
| 57.63 | 606.64 | 84.40 | 1002.84 | -13.01 | 166.31 | -69.13 | 104.67 | 0.9426 | 496.4 | -186.5 | |
| 1.29 | -2.00 | 2.43 | -2.00 | -14.23 | 161.72 | -73.72 | 105.38 | 0.9662 | -559.9 | 999999 | |
| 5.49 | -2.00 | 10.53 | -2.00 | -13.99 | 161.49 | -73.95 | 105.11 | 0.9671 | -611.9 | 999999 | |
| 8.49 | -2.00 | 17.56 | -2.00 | -14.68 | 160.37 | -75.07 | 105.70 | 0.9720 | -222.5 | 999999 | |
| 0.00 | 0.34 | 0.00 | 0.69 | -14.23 | 160.68 | -74.76 | 105.28 | 0.9706 | -276.0 | -263.8 | |
| 0.00 | 0.69 | 0.00 | 1.38 | -13.96 | 160.71 | -74.73 | 105.00 | 0.9704 | -492.0 | -412.2 | |
| 1.37 | -2.00 | 2.88 | -2.00 | -14.23 | 160.09 | -75.35 | 105.21 | 0.9729 | 138.2 | 999999 | |
| 2.57 | -2.00 | 5.71 | -2.00 | -14.74 | 159.42 | -76.02 | 105.67 | 0.9757 | 147.9 | 999999 | |
| 0.00 | 1.54 | 0.00 | 3.25 | -13.86 | 160.08 | -75.36 | 104.83 | 0.9728 | -240.0 | -112.1 | |
| 0.00 | 0.43 | 0.00 | 0.81 | -12.15 | 161.55 | -73.89 | 103.23 | 0.9660 | -414.0 | -382.4 | |
| 0.00 | 1.72 | 0.00 | 3.88 | -14.42 | 159.12 | -76.32 | 105.31 | 0.9766 | 223.0 | 251.8 | |
| 0.69 | 2.32 | 1.62 | 5.48 | -14.13 | 158.49 | -76.95 | 104.96 | 0.9788 | -77.9 | -28.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |